. Recent work on solar wind plasma correlations using data from several widely#separated spacecraft #IMP 8# INTERBALL#1# WIND# and ISEE#3# has shown that# for 6#hour periods# the average plasma correlation is #0.7. The focus of these studies has been directed toward a statistical understanding of gross solar wind correlation behavior. In all correlations examined# lower average correlations are caused by the presence of many points from the low correlation subpopulation# nevertheless# data points from the high correlation population are still present. No single organizational factor has yet been found which adequately separates low#correlation periods from high#correlation periods. Some of the spread in correlations is due to the s...
A novel multi-spacecraft technique, applied to measurements made by the four Cluster spacecraft in t...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95101/1/jgra21350.pd
A brief review of typical features of the variations in the solar wind parameters (plasma and magnet...
Proton velocity data from identical plasma instruments on board NASA\u27s two Stereo spacecraft are ...
We investigate the spatial correlation properties of the solar wind in the ecliptic at 1 AU using si...
We present the results of a study of solar wind velocity and magnetic field correlation lengths over...
We present the results of a study of solar wind velocity and magnetic field correlation lengths over...
We present the results of a study of solar wind velocity and magnetic field correlation lengths over...
Single point measurement turbulence cannot distinguish variations in space and time. We employ an en...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
By using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explorer), a statistical st...
Simultaneous multiple point measurements of the magnetic field from 11 spacecraft are employed to de...
Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only dir...
A novel multi-spacecraft technique, applied to measurements made by the four Cluster spacecraft in t...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95101/1/jgra21350.pd
A brief review of typical features of the variations in the solar wind parameters (plasma and magnet...
Proton velocity data from identical plasma instruments on board NASA\u27s two Stereo spacecraft are ...
We investigate the spatial correlation properties of the solar wind in the ecliptic at 1 AU using si...
We present the results of a study of solar wind velocity and magnetic field correlation lengths over...
We present the results of a study of solar wind velocity and magnetic field correlation lengths over...
We present the results of a study of solar wind velocity and magnetic field correlation lengths over...
Single point measurement turbulence cannot distinguish variations in space and time. We employ an en...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
International audienceBy using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explor...
By using the data of two spacecraft, TC-1 and ACE (Advanced Composition Explorer), a statistical st...
Simultaneous multiple point measurements of the magnetic field from 11 spacecraft are employed to de...
Interplanetary turbulence, the best studied case of low frequency plasma turbulence, is the only dir...
A novel multi-spacecraft technique, applied to measurements made by the four Cluster spacecraft in t...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95101/1/jgra21350.pd
A brief review of typical features of the variations in the solar wind parameters (plasma and magnet...